Search Results - "Davoult, J"

Confronting compositional confusion through the characterization of the sub-Neptune orbiting HD 77946 by Palethorpe, L, Anna John, A, Mortier, A, Davoult, J, Wilson, T G, Rice, K, Cameron, A C, Alibert, Y, Buchhave, L A, Malavolta, L, Cadman, J, López-Morales, M, Dumusque, X, Silva, A M, Quinn, S N, Van Eylen, V, Vissapragada, S, Affer, L, Charbonneau, D, Cosentino, R, Ghedina, A, Haywood, R D, Latham, D W, Lienhard, F, Fiorenzano, A F Martínez, Pedani, M, Pepe, F, Pinamonti, M, Sozzetti, A, Stalport, M, Udry, S, Vanderburg, A

“…ABSTRACT We report on the detailed characterization of the HD 77946 planetary system. HD 77946 is an F5 (M*  = 1.17 M⊙, R*  = 1.31 R⊙) star, which hosts a…”
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Confronting compositional confusion through the characterisation of the sub-Neptune orbiting HD 77946 by Palethorpe, L, John, A. Anna, Mortier, A, Davoult, J, Wilson, T. G, Rice, K, Cameron, A. C, Alibert, Y, Buchhave, L. A, Malavolta, L, Cadman, J, López-Morales, M, Dumusque, X, Silva, A. M, Quinn, S. N, Van Eylen, V, Vissapragada, S, Affer, L, Charbonneau, D, Cosentino, R, Ghedina, A, Haywood, R. D, Latham, D. W, Lienhard, F, Fiorenzano, A. F. Martínez, Pedani, M, Pepe, F, Pinamonti, M, Sozzetti, A, Stalport, M, Udry, S, Vanderburg, A

“…MNRAS, 529, 3323-3341 (2024) We report on the detailed characterization of the HD 77946 planetary system. HD 77946 is an F5 ($M_*$ = 1.17 M$_{\odot}$, $R_*$ =…”
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A compact multi-planet system transiting HIP 29442 (TOI-469) discovered by TESS and ESPRESSO. Radial velocities lead to the detection of transits with low signal-to-noise ratio by Damasso, M, Rodrigues, J, Castro-González, A, Lavie, B, Davoult, J, Osorio, M. R. Zapatero, Dou, J, Sousa, S. G, Owen, J. E, Sossi, P, Adibekyan, V, Osborn, H, Leinhardt, Z, Alibert, Y, Lovis, C, Mena, E. Delgado, Sozzetti, A, Barros, S. C. C, Bossini, D, Ziegler, C, Ciardi, D. R, Matthews, E. C, Carter, P. J, Lillo-Box, J, Mascareño, A. Suárez, Cristiani, S, Pepe, F, Rebolo, R, Santos, N. C, Prieto, C. Allende, Benatti, S, Bouchy, F, Briceño, C, Di Marcantonio, P, D'Odorico, V, Dumusque, X, Egger, J. A, Ehrenreich, D, Faria, J, Figueira, P, Santos, R. Génova, Gonzales, E. J, Hernández, J. I. González, Law, N, Curto, G. Lo, Mann, A. W, Martins, C. J. A. P, Mehner, A, Micela, G, Molaro, P, Nunes, N. J, Palle, E, Poretti, E, Schlieder, J. E, Udry, S

“…We followed-up with ESPRESSO the K0V star HIP 29442 (TOI-469), already known to host a validated sub-Neptune companion TOI-469.01. We aim to verify the…”
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An unusually low-density super-Earth transiting the bright early-type M-dwarf GJ 1018 (TOI-244) by Castro-González, A, Demangeon, O. D. S, Lillo-Box, J, Lovis, C, Lavie, B, Adibekyan, V, Acuña, L, Deleuil, M, Aguichine, A, Osorio, M. R. Zapatero, Tabernero, H. M, Davoult, J, Alibert, Y, Santos, N, Sousa, S. G, Antoniadis-Karnavas, A, Borsa, F, Winn, J. N, Prieto, C. Allende, Figueira, P, Jenkins, J. M, Sozzetti, A, Damasso, M, Silva, A. M, Astudillo-Defru, N, Barros, S. C. C, Bonfils, X, Cristiani, S, Di Marcantonio, P, Hernández, J. I. González, Curto, G. Lo, Martins, C. J. A. P, Nunes, N. J, Palle, E, Pepe, F, Seager, S, Mascareño, A. Suárez

“…A&A 675, A52 (2023) Small planets located at the lower mode of the bimodal radius distribution are generally assumed to be composed of iron and silicates in a…”
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